Elizabeth Howell, Author at Universe Today

February 12, 2014December 23, 2015 by Elizabeth Howell

What Is NASA For? Space Enthusiasts Fight For Agency’s Reputation On Twitter

The International Space Station. Credit: NASA

A week ago today, Slate published an article asking “What Is NASA for?” After the author opened the article comparing the United States’ space agency to a panda, he described a sort of loss of direction that fell upon NASA after the moon landings concluded in 1972. He then cited a litany of concerns he has about the agency, including human spaceflight scientific results not appearing in top journals, and the cost of the International Space Station.

Then Twitter space fans responded with a flurry of tweets under the hashtag #WhatIsNASAFor (3,994 tweets and retweets according to this graph cited by NASA Watch). Participants included NASA officials, journalists, industry and people who follow NASA and space exploration as a hobby. Several people also wrote essays in longer form (such as Deep Space Industries’ Rick Tumlinson, who argued the agency is in the middle of a paradigm shift). Below, we’ve collected some of the most interesting responses from Twitter.

Predicting climate change

Virginia’s Angela Gibson, who says in her profile that she has attended NASA Socials in the past, points to NASA’s ability to do scientific work to better understand climate change. She pointed to this animation of 2013’s warming trend as an example.

Scientific inquiry and the human spirit

As always, Bad Astronomy’s Phil Plait writes an eloquent essay talking about the benefits of NASA, which range from real-time observations of the Earth’s immediate environment to the longer-term goals of promoting scientific research.

NASA Socials

Frequent NASA Social attendee Charissa S. talks about the first NASA launch tweetup, STS-129, as a part of why NASA means so much to her. (Full disclosure: this article’s author also attended the tweetup as a reporter.)

International collaboration

We at Universe Today frequently write about the stunning images from the Mars Reconnaissance Orbiter’s High Resolution Imaging Science Experiment (HiRISE). The HiRISE social media feeds are, thanks to volunteer effort, available in many languages, something they highlighted in a tweet.

Then there’s also the technical potential of nations working together, as feed OH, Star Stuff points out.

Career potential

NASA spokesperson Trent Perrotto talked about a long-ago trip to NASA Johnson that made him see the possibilities of working in space.

And speaking of human potential, the Challenger Center’s Libby Norcross has perhaps the best retort ever by way of Tsiolkovsky.

February 11, 2014December 23, 2015 by Elizabeth Howell

Music Video From Saturn Shows Off Dazzling Aurora Light Show

An aurora around Saturn's north pole in 2013. Credit: NASA/ESA/University of Leicester and NASA/JPL-Caltech/University of Arizona/Lancaster University

Above is the latest rave-like video from NASA. While the images are reminiscent of what could play during an awesome Friday night party, what you’re actually seeing is a timelapse of auroras on Saturn. These pictures are pretty to look at, but they also tell us more about how the sun’s belches of stuff influence the magnetic field around the ringed gas giant.

“Saturn’s auroras can be fickle — you may see fireworks, you may see nothing,” stated Jonathan Nichols of the University of Leicester in England, who led the work on the Hubble Space Telescope images shown in the video. “In 2013, we were treated to a veritable smorgasbord of dancing auroras, from steadily shining rings to super-fast bursts of light shooting across the pole.”

The light show was captured by both the Saturn-orbiting Cassini spacecraft and the Earth-orbiting Hubble. Cassini managed to nab its images from three Saturn distances away (which is apparently an unusually close vantage point.) This location “provided a look at the changing patterns of faint emissions on scales of a few hundred miles (kilometers) and tied the changes in the auroras to the fluctuating wind of charged particles blowing off the sun and flowing past Saturn,” NASA stated.

Here are a few things scientists are learning (or hoping to learn soon) from the light show:

How auroras are formed. The Cassini images suggest that as magnetic field lines forge new links, this is where the storms are centered. This process happens on Earth, so it would make sense for it to happen elsewhere. Researchers also found that some of the auroras stick close to the orbital position of Mimas, suggesting that the moon may be influencing some of the storms (a process already known to happen with Enceladus).
The nature of Saturn’s atmosphere. While the answers are still forthcoming, scientists are examining why the top of Saturn’s atmosphere (and other gas giants) are warmer than would be expected given how far they are from the sun. “By looking at these long sequences of images taken by different instruments, we can discover where the aurora heats the atmosphere as the particles dive into it and how long the cooking occurs,” stated Sarah Badman, a Cassini visual and infrared mapping spectrometer team associate at Lancaster University, England.
What color the auroras are. Red on the bottom, and purple on the top, depending on how Saturn’s hydrogen is excited and what light it emits. (For reference, Earth’s is green on bottom and red at top due to excitement of nitrogen and oxygen).
Where charged particles around Saturn go. More data from the W.M. Keck Observatory and NASA’s Infrared Telescope Facility (both in Hawaii) could show “how particles are ionized in Saturn’s upper atmosphere,” NASA stated. Better yet, scientists can compare that information to the stuff gathered from outside of Earth’s atmosphere by Hubble and Cassini. This will allow them to see what distortions the ground-based observatories experienced due to Earth’s atmosphere, and improve the accuracy of the observations.

Not bad work for a single music video, isn’t it? For more information on auroras on Saturn, check out these past Universe Today stories:

Source: NASA Jet Propulsion Laboratory

February 11, 2014December 23, 2015 by Elizabeth Howell

Google Subsidiary To Negotiate For Giant Eight-Acre NASA California Facility, Hangar One

A 1999 image of Hangar 1 taken in Moffett Field, Calif. Credit: NASA Ames Research Center

Back in late 2011, three Google executives reportedly approached NASA because they knew the agency was facing a problem. NASA was managing the eight-acre Hangar One, which is best remembered for being an airship construction facility 80 years ago. Renovations were getting expensive, though, and the executives had a proposal: it would take over the fixing-up, as long as they could park several private jets in the facility.

Fast-forward a couple of years, and after a competitive process Google real estate subsidiary Planetary Ventures LLC is going to negotiate on a lease with two goals: fix up Hangar One and manage Moffett Federal Airfield. If approved, the lease would remove the NASA Ames Research Center’s management costs.

It’s another example of NASA looking to lease out its historic facilities to the private sector (examples: here and here) to save money amid cost-consciousness by federal legislators, something that administrator Charles Bolden highlighted in a statement. “The agreement announced today will benefit the American taxpayer and the community around Moffett,” he said. “It will allow NASA to focus its resources on core missions, while protecting the federal need to use Moffett Field as a continued, limited-use airfield.”

An undated photo showing a blimp inside Hangar One. The facility began as a facility for airships in the 1930s. Credit: NASA Ames Research Center

Lease terms are still being negotiated, but these are some of the things expected to be a part of it: rehabilitating Hangars One, 2 and 3, fixing up a golf course, starting a public use and educational facility, and getting rid of NASA’s operation and maintenance cost of the area, among other things. In a press release, NASA did not give a date as to when these negotiations would conclude.

As Wired points out, this is an indication that Google and NASA are becoming trusted partners in ventures such as this. “It underscores the increasingly tight relationship between Google and the space agency research center, located just three miles from Google’s headquarters,” wrote Robert McMillan. “Google has already leased more than 40 acres of NASA Ames space to build a 1.2-million-square-foot R&D facility, and the company is working with NASA to test the world’s first quantum computer at Ames too.”

You can read the request for proposals and other information on Hangar One at this NASA website.

February 11, 2014December 23, 2015 by Elizabeth Howell

Saturn’s Ring Shows A Twist In Cassini’s Glimpse Of Planet

Saturn's F ring appears distorted in this October 2013 picture from the Cassini spacecraft. The twisting may be because the F ring is crashing repeatedly into a "single small object", NASA stated. Credit: NASA/JPL-Caltech/Space Science Institute

What’s up with this distortion? This picture from the Cassini spacecraft shows some kind of twist happening in the F ring of Saturn. Scientists in fact have seen other strange shapes in this delicate ring, indicating that something is disturbing it from time to time.

“Saturn’s F ring often appears to do things other rings don’t. In this Cassini spacecraft image, a strand of ring appears to separate from the core of the ring as if pulled apart by mysterious forces. Some ring scientists believe that this feature may be due to repeated collisions between the F ring and a single small object,” NASA stated this month.

There’s a debate in the scientific community about where the rings arose in the first place. “It’s been going back and forth for ages and it still goes back and forth. Are they old, or have they been there a long period of time? Are they new? I don’t know what to think, to be quite honest. I’m not being wishy-washy, I just don’t know what to think anymore,” Kevin Grazier, a planetary scientist with the Cassini mission for over 15 years, told Universe Today in December.

While this picture dates from October, you can check out Cassini images as they come in to NASA’s raw image database. Even in unprocessed form, the planet and its rings look beautiful — as you can clearly see in samples below.

The bulk of Saturn looms to the side of this shot of Saturn's rings taken in February 2014 by the Cassini spacecraft. Credit: NASA/JPL/Space Science Institute — The bulk of Saturn looms to the side of this shot of Saturn’s rings taken in February 2014 by the Cassini spacecraft. Credit: NASA/JPL/Space Science Institute

The variety of Saturn's rings is visible in this raw shot from the Cassini spacecraft taken in February 2014. Credit: NASA/JPL/Space Science Institute — The variety of Saturn’s rings is visible in this raw shot from the Cassini spacecraft taken in February 2014. Credit: NASA/JPL/Space Science Institute

Although Saturn's rings look solid and substantial in images such as this, they are made up of many tiny, icy objects collecting as thin as 6.2 miles (10 kilometers) deep. Image taken by the Cassini spacecraft in February 2014. Credit: NASA/JPL/Space Science Institute — Although Saturn’s rings look solid and substantial in images such as this, they are made up of many tiny, icy objects collecting as thin as 6.2 miles (10 kilometers) deep. Image taken by the Cassini spacecraft in February 2014. Credit: NASA/JPL/Space Science Institute

February 10, 2014December 23, 2015 by Elizabeth Howell

How Massive Is A Neutrino? Cosmology Experiment Gives A Clue

Artist's conception of Planck, a space observatory operated by the European Space Agency, and the cosmic microwave background. Credit: ESA and the Planck Collaboration - D. Ducros

There have been a lot of attempts over the years to figure out the mass of a neutrino (a type of elementary particle). A new analysis not only comes up with a number, but also combines that with a new understanding of the universe’s evolution.

The research team investigated the mass further after observing galaxy clusters with the Planck observatory, a space telescope with the European Space Agency. As the researchers examined the cosmic microwave background (the afterglow of the Big Bang), they saw a difference between their observations and other predictions.

“We observe fewer galaxy clusters than we would expect from the Planck results and there is a weaker signal from gravitational lensing of galaxies than the CMB would suggest. A possible way of resolving this discrepancy is for neutrinos to have mass. The effect of these massive neutrinos would be to suppress the growth of dense structures that lead to the formation of clusters of galaxies,” the researchers stated.

The HST WFPC2 image of gravitational lensing in the galaxy cluster Abell 2218, indicating the presence of large amount of dark matter (credit Andrew Fruchter at STScI).

Neutrinos are a tiny piece of matter (along with other particles such as quarks and electrons). The challenge is, they’re hard to observe because they don’t react very easily to matter. Originally believed to be massless, newer particle physics experiments have shown that they do indeed have mass, but how much was not known.

There are three different flavors or types of neutrinos, and previous analysis suggested the sum was somewhere above 0.06 eV (less than a billionth of a proton’s mass.) The new result suggests it is closer to 0.320 +/- 0.081 eV, but that still has to be confirmed by further study. The researchers arrived at that by using the Planck data with “gravitational lensing observations in which images of galaxies are warped by the curvature of space-time,” they stated.

“If this result is borne out by further analysis, it not only adds significantly to our understanding of the sub-atomic world studied by particle physicists, but it would also be an important extension to the standard model of cosmology which has been developed over the last decade,” the researchers stated.

The research was done by the University of Manchester’s Richard Battye and the University of Nottingham’s Adam Moss. A paper on the work is published in Physical Review Letters and is also available in preprint version on Arxiv.

February 10, 2014December 23, 2015 by Elizabeth Howell

Are These Water Flows On Mars? Quite Possibly, New Observations Reveal

Palikir Crater as seen by the Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (HiRISE) camera. Visible are warm-season flows called "recurring slope linea" that could have been created by salty liquid water. Credit: NASA/JPL-Caltech/UA/JHU-APL

What a tangled web of water and water ice stories on Mars. There’s likely some underground. There’s definitely some at the north pole. And we are pretty certain water flowed there in the ancient past. But what about surface water today, right now, in the view of our many orbiting cameras at the Red Planet?

One hotspot of debate are flows called “recurring slope lineae”, which are features that appear in warmer temperatures. These would seem to imply some kind of briny water flowing. A team recently checked out 13 of these sites. While they didn’t find any water or salt evidence in the spectra, they did find more iron-bearing minerals on “RSL slopes” compared to those that aren’t. So what’s going on?

“We still don’t have a smoking gun for existence of water in RSL, although we’re not sure how this process would take place without water,” stated Lujendra Ojha, a graduate student at the Georgia Institute of Technology in Atlanta who led two reports on these features. Pictures were taken using NASA’s Mars Reconnaissance Orbiter’s High Resolution Imaging Science Experiment (HiRISE), which is led by the University of Arizona.

It’s possible that the grains are being sorted by size (more plainly speaking, taking the fine dust away and leaving the larger grains behind), which could happen either with water or without it. Or, water might be present but not in a way that is obvious immediately if the area got darker because of moisture, or the minerals became oxidized. Water could be “missing” from these observations because they took place in the afternoon (meaning they could miss morning dew), or because the dark flows are smaller than the sample size in the picture.

While researchers still aren’t sure, the team says they still believe it’s salty water of some sort that is flowing despite very cold temperatures on Mars.

“The flow of water, even briny water, anywhere on Mars today would be a major discovery, impacting our understanding of present climate change on Mars and possibly indicating potential habitats for life near the surface on modern Mars,” said Richard Zurek, MRO project scientist who is at NASA’s Jet Propulsion Laboratory in California.

A related paper also found that RSL sites are rare on Mars, appearing in only 13 of 200 sites surveyed with similar slopes, latitudes and other features. You can read the accepted versions of the reports as they appear in Geophysical Research Letters and Icarus.

February 10, 2014December 23, 2015 by Elizabeth Howell

50 Years After Taking Over Earth, The Beatles’ Space Invasion Is Well Underway

Credit: Inside Science News Service and Amanda Page

As the Beatles strummed the opening notes to “All My Loving” on the Ed Sullivan Show 50 years ago yesterday, few could have imagined how wide-ranging that music would be. The broadcast gave birth to a global music phenomenon. And like all TV broadcasts of the day, the music carried out into space at the speed of light.

The Inside Science infographic above (see below for the full version) traces the history of the Beatles in relation to how far the broadcast travelled in that time. While those waves were washing out, er, across the universe, the Beatles have been taking over human space exploration in other ways. Below the jump are seven of the more memorable moments.

Rocking The Space Station With ‘Back at the ISS’

Technically speaking, this isn’t the Beatles, but it sure was inspired by them. ‘Back at the ISS’ — the remake of ‘Back in the U.S.S.R.’ by Dutch band Love & Mersey — is about a billion shades of awesome. Not only because of the lyrics, not only because of the high-energy space-themed video, but also because they sang in three languages. The song was released in March 2012 as a “rocking musical greeting” to Andre Kuipers (a European Space Agency astronaut) and the rest of the Expedition 30 crew days before the docking of the Automated Transfer Vehicle Edoardo Amaldi that month.

Beatles In The Sky With … Asteroids

Yup, there’s an asteroid named after the Beatles. Oh yeah, there are also asteroids named after members John Lennon, Paul McCartney, George Harrison and Ringo Starr.

Good Morning Good Morning wake-up calls

The Beatles have been used to wake up several shuttle crews, and also the Curiosity rover. Explained Eric Blood, Curiosity’s surface systems engineer: “She tends to be less cranky with a good wakeup song.”

Playing (And Drinking?) English Tea In Space

Here’s Paul McCartney in 2005 casually playing two tunes to the Expedition 12 crew — NASA astronaut Bill McArthur and Russian cosmonaut Valery Tokarev — during a live concert. It’s a bit hard to tell who had bigger stars in their eyes after the experience. “I told the audience ‘I think I need about 20 minutes to go have a lie down,’ McCartney stated in a NASA release from the time. “What do you do after that? We haven’t stopped talking about it since.”

Roll Over Beethoven: How The Beatles Almost Made Voyager’s ‘Golden Record’

Remember when scientists announced last year that Voyager 1 entered interstellar space? On board the spacecraft was a Golden Record intended to give aliens a glimpse into what Earth’s life is like. Included were songs from artists ranging from Bach to Blind Willie Johnson, but not the Beatles. They were almost included, though, as astronomer Carl Sagan (who chaired the selection committee) explained in his 1978 book Murmers of Earth. “We wanted to send ‘Here Comes The Sun’ by the Beatles, and all four Beatles gave their approval. But the Beatles did not own the copyright, and the legal status of the piece seemed too murky to risk,” he wrote.

Joining Mr. Mercury’s Light

There are so many earthly memorials to John Lennon after the singer’s untimely death in 1980, but late last year he got an extraterrestrial honor. Lennon was among 10 names approved for craters on the planet Mercury. “It’s unlikely that Mercury’s surface is populated with tangerine trees and marmalade skies, but the famous British musician who coined that phrase now has a physical presence on the planet closest to the Sun,” NASA said.

Sending Love To The Aliens With Jai Guru Deva Om

February 4, 2008 marked the first time NASA beamed any song into deep space, and what better choice than “Across The Universe”? The date marked the 40th anniversary of when the Beatles recorded the song, and came around the same time as the 45th anniversary of NASA’s Deep Space Network and the 50th anniversary of NASA’s first satellite, Explorer 1, among other milestones. In a statement, McCartney asked to “send my love to the aliens.”

What Beatles milestones in space have we missed? Let us know in the comments.

February 10, 2014December 23, 2015 by Elizabeth Howell

Found! Distant Galaxy Spotted Just 650 Million Years After Big Bang

Hubble Space Telescope deep image of galaxy cluster Abell 2744. Credit: NASA, ESA, J. Lotz, M. Mountain, A. Koekemoer, and the HFF Team (STScI), and N. Laporte (Instituto de Astrofisica de Canarias)

Peering deep into the universe with the Hubble Space Telescope, a team of researchers have found an extremely distant galaxy. It was discovered in Abell 2744, a galaxy cluster. The galaxy (called Abell2744_Y1) was spotted at a time when it was just 650 million years after the universe-forming Big Bang (which makes it more than 13 billion years old).

This demonstrates the potential of a relatively new project, researchers said, called “Hubble Frontier Fields.” It’s part of an effort where Hubble and fellow NASA space telescopes Spitzer and the Chandra X-ray Observatory will examine six galaxy clusters that bend the light from more distant objects in the background. By doing this, researchers hope to learn more about galaxies formed in the universe’s first billion years.

“We expected to find very distant galaxies close to the cluster core, where the light amplification is maximum. However, this galaxy is very close to the edge of the Hubble image where the light is not strongly amplified,” stated Nicolas Laporte, a post-doctoral researcher at the Institute of Astrophysics of the Canary Islands (Instituto de Astrofisica de Canarias) who led the study.

“We are really lucky that we could find it in the small field of view of Hubble. In a related study led by Hakim Atek … more galaxies are analyzed but none is more distant than Abell2744_Y1.”

You can read the study in the journal Astronomy and Astrophysics Letters or in preprint version on Arxiv.

Source: Space Telescope Science Institute and Institute of Astrophysics of the Canary Islands

February 7, 2014April 26, 2016 by Elizabeth Howell

Kapow! Black Hole’s Jet Highlights A Galactic ‘Dust Lane’ 12 Million Light-Years Away

Centaurus A (the site of a supermassive black hole) shines brightly in this composite image from the Chandra X-ray Observatory. Scientists used the equivalent of 9.5 days' worth of observations between 1999 and 2012. Credit: X-ray: NASA/CXC/U.Birmingham/M.Burke et al.

This image, right here, shows us the value of long-term observations. It’s a composite of pictures taken between 1999 and 2012 from NASA’s Chandra X-ray Telescope. Put 9.5 days’ worth of observations together, and you can see a lot of action in Centaurus A — namely, a huge jet emanating from a ginormous black hole embedded in the galaxy.

“As in all of Chandra’s images of Cen A, this one shows the spectacular jet of outflowing material – seen pointing from the middle to the upper left – that is generated by the giant black hole at the galaxy’s center. This new high-energy snapshot of Cen A also highlights a dust lane that wraps around the waist of the galaxy. Astronomers think this feature is a remnant of a collision that Cen A experienced with a smaller galaxy millions of years ago,” NASA stated.

Black hole with disc and jets visualization courtesy of ESA

A past survey of X-ray sources in Cen A revealed that most of them are black holes or neutron stars (the latter created from the wake of a huge star’s collapse). It seems that most of these sources are either less than twice the mass of the sun, or more than five times as massive. Here’s the more interesting bit: the smaller ones appear to be neutron stars, and the bigger ones black holes.

“This mass gap may tell us about the way massive stars explode. Scientists expect an upper limit on the most massive neutron stars, up to twice the mass of the Sun,” NASA added.

“What is puzzling is that the smallest black holes appear to weigh in at about five times the mass of the Sun. Stars are observed to have a continual range of masses, and so in terms of their progeny’s weight we would expect black holes to carry on where neutron stars left off.”

The 2013 paper is available both in The Astrophysical Journal and in preprint version on Arxiv.

February 7, 2014December 23, 2015 by Elizabeth Howell

How A Laser Appears To Move Faster Than Light (And Why It Really Isn’t)

Gieren et al. used the 8.2-m Very Large Telescope (Yepun) to image M33, and deduce the distance to that galaxy (image credit: ESO).

We at Universe Today often hear theories purporting that Einstein is wrong, and perhaps one of the most common things cited is the speed limit for light used in his relativity theories. In a vacuum, light goes close to 300,000 km/s (roughly 186,000 miles a second). Using a bit of geometry, however, isn’t there a way to make it go faster? This video below shows why you’d think it would work that way, but it actually wouldn’t.

“There is a classic method where you shine a laser at the moon. If you can flick that beam across the moon’s surface in less than a hundredth of a second, which is not hard to do, then that laser spot will actually move across the surface of the moon faster than the speed of light,” says the host on this Veritasium video.

“In truth, nothing here is really travelling faster than the speed of light. The individual particles coming out of my laser, the photons, are still travelling to the moon at the speed of light. It’s just that they’re landing side by side in such quick succession that they form a spot that moves faster than the speed of light, but really, it’s just an illusion.”

There are way more ways that light can appear to move faster than the cosmic video, and you can check out more of those in the video.